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Fig. A.1

image

Flux (left panels), squared visibility amplitudes (middle panels), and closure phases (right panels) of R Cnc from data sets no. 1 to 6 (top to bottom) of Table 1 (black lines). Also shown are model predictions from the best-fit 1D CODEX (blue lines) and 3D CO5BOLD (red lines) models from Table 3. The squared visibility amplitudes include three lines that correspond to the three baselines of each AMBER dataset. Mean error bars are drawn in the center of each third of the total wavelength range. In particular, for the logarithmic scales, these are sometimes too small to be easily visible. They are typically 5–20% for the fluxes, 5–15% for the squared visibility amplitudes, and 5–15 deg for the closure phases.

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